\begin{document}$ {\cal{S}}$\end{document} with non-trivial \begin{document}$ B-L$\end{document} charges in the conformal \begin{document}$ U(1)_{B-L}$\end{document} theory. It was found that, in a sizable region of parameter space, \begin{document}$ {\cal{S}}$\end{document} may disturb the resonant leptogenesis mechanism, which is used to generate baryon asymmetry, and affect the symmetry breaking dynamics in the strong first order phase transition. The stochastic gravitational waves (GWs) produced at the phase transition can be probed in future GW experiments. The GW searches prefer a relatively light \begin{document}$ {\cal{S}}$\end{document} at the TeV-scale; however, this is difficult to detect directly at future high-energy colliders."> Cosmological implications of a <i>B</i> − <i>L</i> charged hidden scalar: leptogenesis and gravitational waves -
  • [1]

    S. R. Coleman and E. J. Weinberg, Phys. Rev. D7, 1888-1910 (1973)

  • [2]

    C. Englert, J. Jaeckel, V. Khozeet al., JHEP04, 060 (2013), arXiv:1301.4224

  • [3]

    A. Farzinnia, H.-J. He, and J. Ren, Phys. Lett. B727, 141-150 (2013), arXiv:1308.0295

  • [4]

    P. Minkowski, Phys. Lett. B67, 421-428 (1977)

  • [5]

    R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett.44, 912 (1980)

  • [6]

    T. Yanagida, Conf. Proc. C7902131, 95-99 (1979)

  • [7]

    M. Gell-Mann, P. Ramond, and R. Slansky, Conf. Proc. C790927, 315-321 (1979), arXiv:1306.4669

  • [8]

    S. Glashow, NATO Sci. Ser. B61, 687 (1980)

  • [9]

    M. Fukugita and T. Yanagida, Phys. Lett. B174, 45-47 (1986)

  • [10]

    V. V. Khoze and G. Ro, JHEP10, 075 (2013), arXiv:1307.3764

  • [11]

    D. Croon, N. Fernandez, D. McKeenet al., JHEP06, 098 (2019), arXiv:1903.08658

  • [12]

    W. Buchmuller, V. Domcke, K. Kamadaet al., JCAP10, 003 (2013), arXiv:1305.3392

  • [13]

    K. Schmitz,The B - L Phase Transition: Implications for Cosmology and Neutrinos. PhD thesis, Hamburg U., 2012. 1307.3887

  • [14]

    W. Buchmuller, V. Domcke, and K. Schmitz, Nucl. Phys. B862, 587-632 (2012), arXiv:1202.6679

  • [15]

    J. Ellis, M. Lewicki, J. M. Noet al., JCAP06, 024 (2019), arXiv:1903.09642

  • [16]

    J. Ellis, M. Lewicki, and J. M. No, JCAP04, 003 (2019), arXiv:1809.08242

  • [17]

    R. Jinno and M. Takimoto, Phys. Rev. D95(1), 015020 (2017), arXiv:1604.05035

  • [18]

    S. Iso, P. D. Serpico, and K. Shimada, Phys. Rev. Lett.119(14), 141301 (2017), arXiv:1704.04955

  • [19]

    W. Chao, H.-K. Guo, and J. Shu, JCAP09, 009 (2017), arXiv:1702.02698

  • [20]

    W. Chao, W.-F. Cui, H.-K. Guoet al.,Gravitational Wave Imprint of New Symmetry Breaking, 1707.09759

  • [21]

    C. Marzo, L. Marzola, and V. Vaskonen, Eur. Phys. J. C79(7), 601 (2019), arXiv:1811.11169

  • [22]

    N. Okada and O. Seto, Phys. Rev. D98(6), 063532 (2018), arXiv:1807.00336

  • [23]

    T. Hasegawa, N. Okada, and O. Seto, Phys. Rev. D99(9), 095039 (2019), arXiv:1904.03020

  • [24]

    P. Amaro-Seoaneet al. (LISA Collaboration),Laser Interferometer Space Antenna, 1702.00786

  • [25]

    T. Robson, N. J. Cornish, and C. Liu, Class. Quant. Grav.36(10), 105011 (2019), arXiv:1803.01944

  • [26]

    W.-H. Ruan, Z.-K. Guo, R.-G. Caiet al.,Taiji Program: Gravitational-Wave Sources, 1807.09495

  • [27]

    J. Luoet al. (TianQin Collaboration), Class. Quant. Grav.33(3), 035010 (2016), arXiv:1512.02076

  • [28]

    V. Corbin and N. J. Cornish, Class. Quant. Grav.23, 2435-2446 (2006), arXiv:gr-qc/0512039

  • [29]

    M. Musha (DECIGO Working group Collaboration), Proc. SPIE Int. Soc. Opt. Eng.10562, 105623T (2017)

  • [30]

    H. Kudoh, A. Taruya, T. Hiramatsuet al., Phys. Rev. D73, 064006 (2006), arXiv:gr-qc/0511145

  • [31]

    T. Hambye, A. Strumia, and D. Teresi, JHEP08, 188 (2018), arXiv:1805.01473

  • [32]

    L. Covi, E. Roulet, and F. Vissani, Phys. Lett. B384, 169-174 (1996), arXiv:hep-ph/9605319

  • [33]

    M. Flanz, E. A. Paschos, U. Sarkaret al., Phys. Lett. B389, 693-699 (1996), arXiv:hep-ph/9607310

  • [34]

    A. Pilaftsis, Phys. Rev. D56, 5431-5451 (1997), arXiv:hep-ph/9707235

  • [35]

    A. Pilaftsis and T. E. Underwood, Nucl. Phys. B692, 303-345 (2004), arXiv:hep-ph/0309342

  • [36]

    S. Blanchet, Z. Chacko, S. S. Granoret al., Phys. Rev. D82, 076008 (2010), arXiv:0904.2174

  • [37]

    S. Blanchet, P. Dev, and R. Mohapatra, Phys. Rev. D82, 115025 (2010), arXiv:1010.1471

  • [38]

    S. Iso, N. Okada, and Y. Orikasa, Phys. Rev. D83, 093011 (2011), arXiv:1011.4769

  • [39]

    N. Okada, Y. Orikasa, and T. Yamada, Phys. Rev. D86, 076003 (2012), arXiv:1207.1510

  • [40]

    J. Heeck and D. Teresi, Phys. Rev. D94(9), 095024 (2016), arXiv:1609.03594

  • [41]

    P. S. B. Dev, R. N. Mohapatra, and Y. Zhang, JHEP03, 122 (2018), arXiv:1711.07634

  • [42]

    D. Akeribet al. (LUX Collaboration), Phys. Rev. Lett.118(2), 021303 (2017), arXiv:1608.07648

  • [43]

    A. Tanet al. (PandaX-Ⅱ Collaboration), Phys. Rev. Lett.117(12), 121303 (2016), arXiv:1607.07400

  • [44]

    X. Cuiet al. (PandaX-Ⅱ Collaboration), Phys. Rev. Lett.119(18), 181302 (2017), arXiv:1708.06917

  • [45]

    E. Aprileet al. (XENON Collaboration), Phys. Rev. Lett.119(18), 181301 (2017), arXiv:1705.06655

  • [46]

    S. Iso, N. Okada, and Y. Orikasa, Phys. Lett. B676, 81-87 (2009), arXiv:0902.4050

  • [47]

    J. Guo, Z. Kang, P. Koet al., Phys. Rev. D91(11), 115017 (2015), arXiv:1502.00508

  • [48]

    W. Rodejohann and C. E. Yaguna, JCAP1512(12), 032 (2015), arXiv:1509.04036

  • [49]

    S. Patra, F. S. Queiroz, and W. Rodejohann, Phys. Lett. B752, 186-190 (2016), arXiv:1506.03456

  • [50]

    M. Lindner, F. S. Queiroz, and W. Rodejohann, Phys. Lett. B762, 190-195 (2016), arXiv:1604.07419

  • [51]

    ATLAS Collaboration,Search for new high-mass resonances in the dilepton final state using proton-proton collisions at \begin{document}$ \sqrt s $\end{document} =13 TeV with the ATLAS detector

  • [52]

    CMS Collaboration,Search for a high-mass resonance decaying into a dilepton final state in 13 fb-1of pp collisions at \begin{document}$ \sqrt s $\end{document} = 13 TeV

  • [53]

    P. Bhupal Dev, R. N. Mohapatra, and Y. Zhang, JHEP11, 077 (2016), arXiv:1608.06266

  • [54]

    N. Okada and O. Seto, Mod. Phys. Lett. A33(27), 1850157 (2018), arXiv:1712.03652

  • [55]

    R. Diener, S. Godfrey, and T. A. Martin, Phys. Rev. D83, 115008 (2011), arXiv:1006.2845

  • [56]

    S. Godfrey and T. Martin,Z’ Discovery Reach at Future Hadron Colliders: A Snowmass White Paper, inCommunity Summer Study 2013: Snowmass on the Mississippi, 9, 2013. 1309.1688

  • [57]

    T. G. Rizzo, Phys. Rev. D89(9), 095022 (2014), arXiv:1403.5465

  • [58]

    V. Khachatryanet al. (CMS Collaboration), Eur. Phys. J. C75(5), 235 (2015), arXiv:1408.3583

  • [59]

    G. Aadet al. (ATLAS Collaboration), Eur. Phys. J. C75(7), 299 (2015) [Erratum: Eur. Phys. J. C75, 408 (2015)], arXiv: 1502.01518

  • [60]

    M. Aaboudet al. (ATLAS Collaboration), JHEP01, 126 (2018), arXiv:1711.03301

  • [61]

    A. M. Sirunyanet al. (CMS Collaboration), Phys. Rev. D97(9), 092005 (2018), arXiv:1712.02345

  • [62]

    S. Davidson and A. Ibarra, Phys. Lett. B535, 25-32 (2002), arXiv:hep-ph/0202239

  • [63]

    K. Moffat, S. Pascoli, S. Petcovet al., Phys. Rev. D98(1), 015036 (2018), arXiv:1804.05066

  • [64]

    B. Dev, M. Garny, J. Klaricet al., Int. J. Mod. Phys. A33, 1842003 (2018), arXiv:1711.02863

  • [65]

    F. F. Deppisch and A. Pilaftsis, Phys. Rev. D83, 076007 (2011), arXiv:1012.1834

  • [66]

    P. S. B. Dev, P. Millington, A. Pilaftsiset al., Nucl. Phys. B897, 749-756 (2015), arXiv:1504.07640

  • [67]

    G. Giudice, A. Notari, M. Raidalet al., Nucl. Phys. B685, 89-149 (2004), arXiv:hep-ph/0310123

  • [68]

    P. Bhupal Dev, P. Millington, A. Pilaftsiset al., Nucl. Phys. B886, 569-664 (2014), arXiv:1404.1003

  • [69]

    M. D’Onofrio, K. Rummukainen, and A. Tranberg, Phys. Rev. Lett.113(14), 141602 (2014), arXiv:1404.3565

  • [70]

    P. Bhupal Dev, C.-H. Lee, and R. Mohapatra, Phys. Rev. D90(9), 095012 (2014), arXiv:1408.2820

  • [71]

    M. Quiros,Finite temperature field theory and phase transitions, inICTP Summer School in High-Energy Physics and Cosmology, pp. 187-259, 1, 1999. hep-ph/9901312

  • [72]

    J. Bernon, L. Bian, and Y. Jiang, JHEP05, 151 (2018), arXiv:1712.08430

  • [73]

    I. Affleck, Phys. Rev. Lett.46, 388 (1981)

  • [74]

    A. D. Linde, Nucl. Phys. B216, 421 (1983) [Erratum: Nucl.Phys. B223, 544 (1983)]

  • [75]

    A. D. Linde, Phys. Lett. B100, 37-40 (1981)

  • [76]

    V. Brdar, A. J. Helmboldt, and J. Kubo, JCAP02, 021 (2019), arXiv:1810.12306

  • [77]

    J. Ellis, M. Lewicki, and J. M. No, JCAP07, 050 (2020), arXiv:2003.07360

  • [78]

    J. Ellis, M. Lewicki, and V. Vaskonen,Updated predictions for gravitational waves produced in a strongly supercooled phase transition, 2007.15586

  • [79]

    C. Capriniet al., JCAP1604(04), 001 (2016), arXiv:1512.06239

  • [80]

    R.-G. Cai, Z. Cao, Z.-K. Guoet al., Natl. Sci. Rev.4, 687-706 (2017), arXiv:1703.00187

  • [81]

    D. J. Weir, Phil. Trans. Roy. Soc. Lond. A376(2114), 20170126 (2018), arXiv:1705.01783

  • [82]

    M. Hindmarsh, S. J. Huber, K. Rummukainenet al., Phys. Rev. Lett.112, 041301 (2014), arXiv:1304.2433

  • [83]

    M. Hindmarsh, S. J. Huber, K. Rummukainenet al., Phys. Rev. D92(12), 123009 (2015), arXiv:1504.03291

  • [84]

    R. Jinno and M. Takimoto,Gravitational waves from bubble dynamics: Beyond the Envelope, 1707.03111

  • [85]

    R. Jinno, S. Lee, H. Seonget al., JCAP11, 050 (2017), arXiv:1708.01253

  • [86]

    R. Jinno and M. Takimoto, Phys. Rev. D95(2), 024009 (2017), arXiv:1605.01403

  • [87]

    D. Cutting, M. Hindmarsh, and D. J. Weir, Phys. Rev. D97(12), 123513 (2018), arXiv:1802.05712

  • [88]

    A. Kosowsky, M. S. Turner, and R. Watkins, Phys. Rev. D45, 4514-4535 (1992)

  • [89]

    A. Kosowsky, M. S. Turner, and R. Watkins, Phys. Rev. Lett.69, 2026-2029 (1992)

  • [90]

    A. Kosowsky and M. S. Turner, Phys. Rev. D47, 4372-4391 (1993), arXiv:astro-ph/9211004

  • [91]

    S. J. Huber and T. Konstandin, JCAP0809, 022 (2008), arXiv:0806.1828

  • [92]

    C. Caprini, R. Durrer, and G. Servant, JCAP0912, 024 (2009), arXiv:0909.0622

  • [93]

    P. Binetruy, A. Bohe, C. Capriniet al., JCAP1206, 027 (2012), arXiv:1201.0983

  • [94]

    J. R. Espinosa, T. Konstandin, J. M. Noet al., JCAP1006, 028 (2010), arXiv:1004.4187

  • [95]

    H.-K. Guo, K. Sinha, D. Vagieet al.,Phase Transitions in an Expanding Universe: Stochastic Gravitational Waves in Standard and Non-Standard Histories, 2007.08537

  • [96]

    M. Hindmarsh and M. Hijazi, JCAP1912(12), 062 (2019), arXiv:1909.10040

  • [97]

    M. Hindmarsh, S. J. Huber, K. Rummukainenet al., Phys. Rev. D96(10), 103520 (2017), arXiv:1704.05871

  • [98]

    C. Capriniet al., JCAP03, 024 (2020), arXiv:1910.13125

  • [99]

    G. D. Moore and T. Prokopec, Phys. Rev. D52, 7182-7204 (1995), arXiv:hep-ph/9506475

  • [100]

    G. D. Moore and T. Prokopec, Phys. Rev. Lett.75, 777-780 (1995), arXiv:hep-ph/9503296

  • [101]

    D. Bodeker and G. D. Moore, JCAP0905, 009 (2009), arXiv:0903.4099

  • [102]

    D. Bodeker and G. D. Moore, JCAP1705(05), 025 (2017), arXiv:1703.08215

  • [103]

    P. J. Steinhardt, Phys. Rev. D25, 2074 (1982)

  • [104]

    A. Kosowsky, A. Mack, and T. Kahniashvili, Phys. Rev. D66, 024030 (2002), arXiv:astro-ph/0111483

  • [105]

    G. Gogoberidze, T. Kahniashvili, and A. Kosowsky, Phys. Rev. D76, 083002 (2007), arXiv:0705.1733

  • [106]

    P. Niksa, M. Schlederer, and G. Sigl, Class. Quant. Grav.35(14), 144001 (2018), arXiv:1803.02271

  • [107]

    A. Roper Pol, S. Mandal, A. Brandenburget al.,Numerical Simulations of Gravitational Waves from Early-Universe Turbulence, 1903.08585

  • [108]

    A. Brandenburg, T. Kahniashvili, S. Mandalet al., Phys. Rev. D96(12), 123528 (2017), arXiv:1711.03804

  • [109]

    V. V. Khoze, C. McCabe, and G. Ro, JHEP08, 026 (2014), arXiv:1403.4953

  • [110]

    A. Biswas, S. Choubey, and S. Khan, JHEP08, 114 (2016), arXiv:1604.06566

  • [111]

    A. Das, N. Okada, and N. Papapietro, Eur. Phys. J. C77(2), 122 (2017), arXiv:1509.01466

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